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A detailed look at the total solar eclipse of March 20, 2015, with detailed path descriptions and viewing circumstances.

A total eclipse of the Sun occurred on Friday 20 March, 2015 UT, lasting from 07:40–11:50 UT. A dramatic total eclipse plunged the Sun into darkness for 2 minutes and 47 seconds at maximum, creating an amazing spectacle for observers in a very broad path, 463 km wide at maximum. It was seen from north-west of the British Isles, including the Faroes. The partial eclipse was visible from Europe, north-west Asia, and north-west Africa.

The timings of the phases of the overall eclipse worldwide are as follows. In any particular place it would have been seen for a significantly shorter duration as the shadow moved across the Earth:

Partial eclipse began: 07:40:52 UT
Total eclipse began: 09:09:33 UT
Maximum eclipse: 09:45:39 UT
Total eclipse ended: 10:21:22 UT
Partial eclipse ended: 11:50:13 UT

During this eclipse the Sun was 0.535° in apparent diameter, 0.4% larger than average. The Moon was at perigee, making it very large. At the start and end of the eclipse the Moon was 0.556°, and at maximum eclipse 0.559°, which is 5.3% larger than average; hence it covered the Sun, making this a total eclipse. The statistics page has information on the ranges of the sizes of the Sun and Moon.


The total eclipse will be visible from the Faroes, but not from the UK. The lucky inhabitants of the Faroes will see the eclipse at about 09:40 UT. On the centreline, the total eclipse will last 2 minutes and 46 seconds; unfortunately, the islands are somewhat south-east of the centre, and will see a shorter eclipse. Still, with the path of totality being 472 km (293.3 miles) wide, they should still see a spectacular eclipse — if the sky is clear. The eclipse reaches its maximum just after it passes the Faroes, at 09:45:38 UT. A 90% partial eclipse will be seen in north-west Scotland, which will still be a significant event.


Svalbard will see the total eclipse between about 10:10 UT and 10:14 UT. The centreline passes over Spitsbergen, but the path of totality covers most of the island group, so the inhabitants (2,642 of them, according to WikipediaSvalbard
Article on Svalbard, which will see a total eclipse on 20 March 2015. Wikipedia
) would be advised to head for a location that gives them their best chance of a clear sky. At 10:12 UT the eclipse will last for 2 minutes and 28 seconds, and the path will be 416 km (258.5 miles) wide; Longyearbyen, very close to the centreline, will see just one second or so less of total eclipse.

Interactive Map

This map shows the visibility of the eclipse. The shaded area saw the total solar eclipse; however, near the edges of this area, the eclipse was very short. The bold line shows the centre of the path, where the eclipse lasted longest.

Use the zoom controls to zoom in and out; hover your mouse over any point on the centreline to see the time and duration of the eclipse at that point. You can pan and zoom the map to see detail for any part of the eclipse path.

Overview Map

This map sourced from NASA Goddard Space flight Center: GSFC Eclipse Web SiteGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. [NASA Goddard Space flight Center]
shows the visibility of the total solar eclipse. It also shows the broader area in which a partial eclipse was seen. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This was the 61st eclipse in solar Saros series 120.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 09:45:38 on 20 Mar UT TDT Date/time (max) 09:46:47 on 20 Mar TDT
Saros Series 120 Number in Series 60
Penumbral Magnitiude Central Magnitiude 1.0445
Gamma 0.9454 Path Width (km) 463
Delta T 1m09s Error ± 0m03s (95%)
Penumbral Duration Partial Duration
Total Duration 2m47s
Partial Rating major Total Rating travel
Sun Distance 148968774 km (38.8%) Moon Distance 357921 km (3.0%)
Sun Diameter 0.535° Moon Diameter 0.556° - 0.559°
Perigee 19:39 on 19 Mar UT Apogee 13:00 on 1 Apr UT
Contact p1 07:40:52 on 20 Mar UT Contact p2
Contact u1 09:09:33 on 20 Mar UT Contact u2 09:16:12 on 20 Mar UT
Max eclipse 09:45:39 on 20 Mar UT
Contact u3 10:14:44 on 20 Mar UT Contact u4 10:21:22 on 20 Mar UT
Contact p3 Contact p4 11:50:13 on 20 Mar UT

Note that while all dates and times on this site (except where noted) are in UT, which is within a second of civil time, the dates and times shown in NASA's eclipse listingsGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. [NASA Goddard Space flight Center]
are in the TDT timescale.

The Sun and Moon distances are shown in km, and as a percentage of their minimum - maximum distances; hence 0% is the closest possible (Earth's perihelion, or the Moon's closest possible perigee) and 100% is the farthest (aphelion, the farthest apogee). The statistics page has information on the ranges of sizes of the Sun and Moon.

Data last updated: 2015-06-21 22:11:46 UTC.